| Evidence for quark-matter cores in massive neutron stars E Annala, T Gorda, A Kurkela, J Nättilä, A Vuorinen Nature Physics 16 (9), 907-910, 2020 | 602 | 2020 |
| Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra J Nättilä, MC Miller, AW Steiner, JJE Kajava, VF Suleimanov, J Poutanen Astronomy & Astrophysics 608, A31, 2017 | 205 | 2017 |
| Multimessenger constraints for ultradense matter E Annala, T Gorda, E Katerini, A Kurkela, J Nättilä, V Paschalidis, ... Physical Review X 12 (1), 011058, 2022 | 138 | 2022 |
| Equation of state constraints for the cold dense matter inside neutron stars using the cooling tail method J Nättilä, AW Steiner, JJE Kajava, VF Suleimanov, J Poutanen Astronomy & Astrophysics 591, A25, 2016 | 138 | 2016 |
| Dense matter with eXTP AL Watts, WF Yu, J Poutanen, S Zhang, S Bhattacharyya, S Bogdanov, ... Science China Physics, Mechanics & Astronomy 62, 1-17, 2019 | 120 | 2019 |
| The effect of accretion on the measurement of neutron star mass and radius in the low-mass X-ray binary 4U 1608− 52 J Poutanen, J Nättilä, JJE Kajava, OM Latvala, DK Galloway, E Kuulkers, ... Monthly Notices of the Royal Astronomical Society 442 (4), 3777-3790, 2014 | 109 | 2014 |
| Combining electromagnetic and gravitational-wave constraints on neutron-star masses and radii M Al-Mamun, AW Steiner, J Nättilä, J Lange, R O’Shaughnessy, I Tews, ... Physical Review Letters 126 (6), 061101, 2021 | 98 | 2021 |
| The influence of accretion geometry on the spectral evolution during thermonuclear (type I) X-ray bursts JJE Kajava, J Nättilä, OM Latvala, M Pursiainen, J Poutanen, ... Monthly Notices of the Royal Astronomical Society 445 (4), 4218-4234, 2014 | 63 | 2014 |
| Strongly interacting matter exhibits deconfined behavior in massive neutron stars E Annala, T Gorda, J Hirvonen, O Komoltsev, A Kurkela, J Nättilä, ... Nature Communications 14 (1), 8451, 2023 | 54 | 2023 |
| Radiation from rapidly rotating oblate neutron stars J Nättilä, P Pihajoki Astronomy & Astrophysics 615, A50, 2018 | 49 | 2018 |
| The direct cooling tail method for X-ray burst analysis to constrain neutron star masses and radii VF Suleimanov, J Poutanen, J Nättilä, JJE Kajava, MG Revnivtsev, ... Monthly Notices of the Royal Astronomical Society 466 (1), 906-913, 2017 | 47 | 2017 |
| Radiative turbulent flares in magnetically dominated plasmas J Nättilä, AM Beloborodov The Astrophysical Journal 921 (1), 87, 2021 | 44 | 2021 |
| Coherent electromagnetic emission from relativistic magnetized shocks L Sironi, I Plotnikov, J Nättilä, AM Beloborodov Physical Review Letters 127 (3), 035101, 2021 | 39 | 2021 |
| Bayesian parameter constraints for neutron star masses and radii using X-ray timing observations of accretion-powered millisecond pulsars T Salmi, J Nättilä, J Poutanen Astronomy & Astrophysics 618, A161, 2018 | 39 | 2018 |
| General purpose ray tracing and polarized radiative transfer in general relativity P Pihajoki, M Mannerkoski, J Nättilä, PH Johansson The Astrophysical Journal 863 (1), 8, 2018 | 38 | 2018 |
| Heating of magnetically dominated plasma by Alfvén-wave turbulence J Nättilä, AM Beloborodov Physical Review Letters 128 (7), 075101, 2022 | 34 | 2022 |
| Observatory science with eXTP JJM in’t Zand, E Bozzo, JL Qu, XD Li, L Amati, Y Chen, I Donnarumma, ... Science China Physics, Mechanics & Astronomy 62, 1-42, 2019 | 34 | 2019 |
| Detection of burning ashes from thermonuclear X-ray bursts JJE Kajava, J Nättilä, J Poutanen, A Cumming, V Suleimanov, E Kuulkers Monthly Notices of the Royal Astronomical Society: Letters 464 (1), L6-L10, 2017 | 32 | 2017 |
| Models of neutron star atmospheres enriched with nuclear burning ashes J Nättilä, VF Suleimanov, JJE Kajava, J Poutanen Astronomy & Astrophysics 581, A83, 2015 | 27 | 2015 |
| Pulsar wind-heated accretion disk and the origin of modes in transitional millisecond pulsar PSR J1023+ 0038 A Veledina, J Nättilä, AM Beloborodov The Astrophysical Journal 884 (2), 144, 2019 | 25 | 2019 |
Juri PoutanenProfessor of Astronomy, University of Turku在 utu.fi 的电子邮件经过验证
